Pulsar interpretation for the AMS-02 result
文献类型：期刊论文
| 作者 | Yin PF(殷鹏飞) ; Yu ZH(余钊焕); Yuan Q(袁强); Bi XJ(毕效军); Yin, PF; Yu, ZH; Yuan, Q; Bi, XJ
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| 刊名 | PHYSICAL REVIEW D
 |
| 出版日期 | 2013 |
| 卷号 | 88期号:2页码:23001 |
| 英文摘要 | The AMS-02 Collaboration has just published a high-precision measurement of the cosmic positron fraction e(+)/(e(-) + e(+)), which rises with energy from similar to 5 GeV to similar to 350 GeV. The result indicates the existence of primary electron/positron sources to account for the positron excess. In this work, we investigate the possibility that the nearby mature pulsars with ages of O(10(5)) yr are the primary positron sources. By fitting the data we find that the positrons from a single nearby pulsar, such as Geminga or Monogem, with the spectral index alpha similar to 2 can interpret the AMS-02 result. We also investigate the possibility that high-energy positrons are generated by multiple known pulsars in the ATNF catalogue. Such a scenario can also fit the AMS-02 data well. Future precise measurements of fine structures in the positron spectrum would be a support to the pulsar scenario. |
| 学科主题 | Astronomy & Astrophysics; Physics |
| 收录类别 | SCI |
| WOS记录号 | WOS:000321208300002 |
| 公开日期 | 2016-05-03 |
| 源URL | [http://ir.ihep.ac.cn/handle/311005/224505]  |
| 专题 | 高能物理研究所_粒子天体物理中心 |
| 推荐引用方式 GB/T 7714 | Yin PF,Yu ZH,Yuan Q,et al. Pulsar interpretation for the AMS-02 result[J]. PHYSICAL REVIEW D,2013,88(2):23001. |
| APA | 殷鹏飞.,余钊焕.,袁强.,毕效军.,Yin, PF.,...&Bi, XJ.(2013).Pulsar interpretation for the AMS-02 result.PHYSICAL REVIEW D,88(2),23001. |
| MLA | 殷鹏飞,et al."Pulsar interpretation for the AMS-02 result".PHYSICAL REVIEW D 88.2(2013):23001. |
入库方式： OAI收割
来源：高能物理研究所
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